slr, grace and swarm gravity field determination and

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Astronomical Institute University of Bern ILRS Workshop Canberra, 05 November 2018 SLR, GRACE and SWARM gravity field determination and combination Ulrich Meyer 1 , Krzysztof Sosnica 2 , Florian Andritsch 1 , Rolf Dach 1 , Adrian Jäggi 1 , Daniel König 3 and Daniela Thaller 3 1 Astronomical Institute, University of Bern, Switzerland 2 Institute of Geodesy and Geoinformatics,Wroclaw University of Environmental and Life Sciences, Poland 3 Bundesamt für Kartographie und Geodäsie, Frankfurt, Germany

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Page 1: SLR, GRACE and SWARM gravity field determination and

Astronomical Institute University of Bern

ILRS Workshop Canberra, 05 November 2018

SLR, GRACE and SWARM gravity field determination and combination

Ulrich Meyer1, Krzysztof Sosnica2, Florian Andritsch1, Rolf Dach1, Adrian Jäggi1, Daniel König3 and

Daniela Thaller3

1Astronomical Institute, University of Bern, Switzerland

2Institute of Geodesy and Geoinformatics,Wroclaw University of Environmental and Life Sciences, Poland

3Bundesamt für Kartographie und Geodäsie, Frankfurt, Germany

Page 2: SLR, GRACE and SWARM gravity field determination and

Slide 2 Astronomical Institute University of Bern

Contents

⚫ Monthly mass variations in Greenland:

▪ SLR

▪ GRACE

▪ SWARM

⚫ Interpretation:

▪ Spatial resolution

▪ Spectral leakage

⚫ Combination of normal equations:

▪ SWARM + SLR

⚫ Summary and Outlook

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Page 3: SLR, GRACE and SWARM gravity field determination and

Slide 3 Astronomical Institute University of Bern

Ice melt in Greenland from SLR

• LAGEOS 1+2: 30 d solutions based on 10 d arcs.• SLR-LEOS (Beacon-C, Ajisai, Starlete, Stella, Larets,

Lares): 30 d solutions based on 1 d arcs.• Gravity field: 5 x 5 + C61 and S61; C50 constrained.• A priori gravity: static 7 y GRACE (AIUB-APR).• A priori orbits: LAGEOS own predictions, LEOS CPF

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Page 4: SLR, GRACE and SWARM gravity field determination and

Slide 4 Astronomical Institute University of Bern

Ice melt in Greenland from GRACE

• GRACE GPS+K-band: monthly 90 x 90 gravity field solutions, truncated at degree / order 6.

• Degree 2 excluded.• Degree 1 fixed to 0.• No filter applied.

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Page 5: SLR, GRACE and SWARM gravity field determination and

Slide 5 Astronomical Institute University of Bern

Ice melt in Greenland from SWARM

• SWARM GPS: monthly 70 x 70 gravity field solutions, truncated at degree / order 6.

• Degree 2 excluded.• Degree 1 fixed to 0.• No filter applied.

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Page 6: SLR, GRACE and SWARM gravity field determination and

Slide 6 Astronomical Institute University of Bern

Spatial resolution and leakage

• The truncation of a spherical harmonic expansion leads to signal leakage.

• Sensitivity for monthly mass variations:• GRACE : 60-90• SWARM: 12-20• SLR: 6-10

• With knowledge about the original mass distribution leakage can be corrected by scaling.

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Page 7: SLR, GRACE and SWARM gravity field determination and

Slide 7 Astronomical Institute University of Bern

Spatial resolution and leakage

• Common filters (e.g. Gauss 300km ) lead to drastic leakage even for GRACE.

• All signal above degree 60, and significant signal above degree 30 is attenuated!

• In case of SLR no filter is applied.

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Page 8: SLR, GRACE and SWARM gravity field determination and

Slide 8 Astronomical Institute University of Bern

Ice mass change: Greenland Coast

• SLR and GRACE provide consistent mass trends when truncated at the same degree / order.

• By scaling, the original amount of mass loss can be recovered almost completely (but not the spatial detail).

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Page 9: SLR, GRACE and SWARM gravity field determination and

Slide 9 Astronomical Institute University of Bern

Ice mass change: Greenland Inland

• Details at small spatial scales are lost. A separation between Greenland coast and inland is not possible with SLR.

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Page 10: SLR, GRACE and SWARM gravity field determination and

Slide 10 Astronomical Institute University of Bern

Combination of NEQs: SWARM + 0.01 * SLR

Contribution analysis per SH

coefficient.

Mean contribution per degree.

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Page 11: SLR, GRACE and SWARM gravity field determination and

Slide 11 Astronomical Institute University of Bern

Combination of NEQs: SWARM + 0.1 * SLR

Contribution analysis per SH

coefficient.

Mean contribution per degree.

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Page 12: SLR, GRACE and SWARM gravity field determination and

Slide 12 Astronomical Institute University of Bern

Combination of NEQs: SWARM + 0.4 * SLR

Contribution analysis per SH

coefficient.

Mean contribution per degree.

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Page 13: SLR, GRACE and SWARM gravity field determination and

Slide 13 Astronomical Institute University of Bern

Combination of NEQs: SWARM + SLR

Contribution analysis per SH

coefficient.

Mean contribution per degree.

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Page 14: SLR, GRACE and SWARM gravity field determination and

Slide 14 Astronomical Institute University of Bern

C20

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• LAGEOS + SLR-LEOs: 30 d C20 values

Page 15: SLR, GRACE and SWARM gravity field determination and

Slide 15 Astronomical Institute University of Bern

C20

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• LAGEOS + SLR-LEOs: 30 d C20 values• GRACE: monthly C20 values, strong correlation with

accelerometer temperature

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Slide 16 Astronomical Institute University of Bern

C20

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• LAGEOS + SLR-LEOs: 30 d C20 values.• GRACE: monthly C20 values, strong correlation with

accelerometer temperature.• SWARM: monthly C20 values (no accelerometers

used for signal separation).

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Slide 17 Astronomical Institute University of Bern

C20

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• LAGEOS + SLR-LEOs: 30 d C20 values.• GRACE: monthly C20 values, strong correlation with

accelerometer temperature.• SWARM: monthly C20 values (no accelerometers

used for signal separation).• SLR + SWARM: C20 dominated by SLR

Page 18: SLR, GRACE and SWARM gravity field determination and

Slide 18 Astronomical Institute University of Bern

C20

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• LAGEOS + SLR-LEOs: 30 d C20 values.• GRACE: monthly C20 values, strong correlation with

accelerometer temperature.• SWARM: monthly C20 values (no accelerometers

used for signal separation).• SLR + SWARM: C20 dominated by SLR• Reference CSR: monthly C20 values for GRACE

Page 19: SLR, GRACE and SWARM gravity field determination and

Slide 19 Astronomical Institute University of Bern

Summary and Outlook

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⚫ Truncated to the same spherical harmonic resolution the three space geodetic techniques SLR, high-low-SST (GPS) and low-low-SST (K-band) provide comparable ice mass trends.

⚫ Taking spectral leakage into account the low resolution SLR mass trends are in agreement with high resolution GRACE results.

⚫ Best SLR + SWARM combination results are achieved with equal weighting.